Abstract
We report on a search for nuclear recoil signals from solar neutrinos elastically scattering off xenon nuclei in XENON1T data, lowering the energy threshold from 2.6 to . We develop a variety of novel techniques to limit the resulting increase in backgrounds near the threshold. No significant neutrinolike excess is found in an exposure of . For the first time, we use the nondetection of solar neutrinos to constrain the light yield from 1–2 keV nuclear recoils in liquid xenon, as well as nonstandard neutrino-quark interactions. Finally, we improve upon world-leading constraints on dark matter-nucleus interactions for dark matter masses between 3 and by as much as an order of magnitude.
- Received 8 December 2020
- Revised 17 January 2021
- Accepted 27 January 2021
DOI:https://doi.org/10.1103/PhysRevLett.126.091301
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society